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Detailed Mass Map of CL 0024+1654 from Strong Lensing

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Tyson, J. Anthony, Kochanski, Greg P., Dell'Antonio, Ian P.·1998·The Astrophysical Journal

DOI 10.1086/311314

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Abstract

We construct a high-resolution mass map of the z =0.39 cluster 0024+1654, based on a parametric inversion of the associated gravitational lens. The lens creates eight well-resolved subimages of a background galaxy, seen in deep imaging with the Hubble Space Telescope . Excluding mass concentrations centered on visible galaxies, more than 98% of the remaining mass is represented by a smooth concentration of dark matter centered near the brightest cluster galaxies, with a 35 h -1 kpc soft core. The asymmetry in the mass distribution is less than 3% inside 107 h -1 kpc radius. The dark matter distribution we observe in CL 0024 is far more smooth, symmetric, and nonsingular than in typical simulated clusters in either Ω=1 or Ω=0.3 cold dark matter cosmologies. Integrated to a 107 h -1 kpc radius, the rest-frame mass-to-light ratio is M / L V =276±40 h (M/L V ) ☉ .

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Authors: Tyson, J. A., Kochanski, G. P., & Dell'Antonio, I. P.
Affiliations: Alcatel-Lucent (France) (FR)
Venue: The Astrophysical Journal
Publisher: American Astronomical Society
Published: 1998-05-10
Volume: 498
Issue: 2
Pages: L107-L110
ISSN: 0004-637X (ISSN-L)
DOI: 10.1086/311314
OpenAlex: W2053222792
Cited by: 335
References: 26
Citations by year: 2026: 3 · 2025: 10 · 2024: 10 · 2023: 4 · 2022: 6 · 2021: 5 · 2020: 6 · 2019: 10 · 2018: 9 · 2017: 8 · 2016: 10 · 2015: 3 · 2014: 11 · 2013: 8 · 2012: 13
FWCI: 18.23
Type: journal article
Language: en
Open access: bronze
doi.org
Locations: The Astrophysical Journal (publishedVersion)
arXiv (Cornell University) (submittedVersion)
CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
arXiv (Cornell University)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
Keywords: galaxy clusters, dark matter distribution, strong gravitational lensing, mass maps, brightest cluster galaxies, soft core, mass-to-light ratio, cluster cosmology, cold dark matter simulations

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Detailed Mass Map of CL 0024+1654 from Strong Lensing

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